Sökning: onr:"swepub:oai:DiVA.org:kth-91583" > Mars Orbiting Plasm...
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000 | 03270naa a2200361 4500 | |
001 | oai:DiVA.org:kth-91583 | |
003 | SwePub | |
008 | 120319s2006 | |||||||||||000 ||eng| | |
024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-915832 URI |
040 | a (SwePub)kth | |
041 | a engb eng | |
042 | 9 SwePub | |
072 | 7 | a vet2 swepub-contenttype |
072 | 7 | a kon2 swepub-publicationtype |
100 | 1 | a Barabash, Stasu Swedish Institute of Space Physics, Kiruna4 aut |
245 | 1 0 | a Mars Orbiting Plasma Surveyor (MOPS) |
264 | 1 | c 2006 |
338 | a electronic2 rdacarrier | |
500 | a QC 20120321 | |
520 | a Mars Orbiting Plasma Surveyor (MOPS) is a microsatellite mission focused on studies of the near -Mars environment and the planet - solar wind interaction. The recent findings by the ESA Mars Express mission further highlighted the complexity of the processes taking place at the planet resulting from the solar wind interaction that strongly affect the planet's atmosphere. However, despite many previous Martian missions carrying different types of space plasma experiments, a comprehensive investigation including simultaneous measurements of particles, fields, and waves has never been performed. We consider a spinning spacecraft of a wet mass of 76.1 kg with a 9.7 kg payload, which can “hitchhike” on another platform until Mars orbit insertion, and then be released into a suitable orbit. The spacecraft design is based on the experience gained in very successful Swedish space plasma missions, Viking, Freja, Astrid-1, and Astrid-2. In the present mission design, the MOPS spacecraft is equipped with its own 1m high gain antenna for direct communication with the Earth. The payload includes a wave experiment with wire booms, magnetometer with a rigid boom, Langmuir probes, electron and ion energy spectrometers and an ion mass analyzer. An energetic neutral atom imager and an UV photometer may complete the core payload. One of the proposed scenarios is piggy - backing on the Russian Phobos - Grunt mission to be launched to Mars in 2011. | |
650 | 7 | a NATURVETENSKAPx Fysikx Fusion, plasma och rymdfysik0 (SwePub)103032 hsv//swe |
650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Fusion, Plasma and Space Physics0 (SwePub)103032 hsv//eng |
700 | 1 | a André, Matsu Swedish Institute of Space Physics, Uppsala4 aut |
700 | 1 | a Blomberg, Larsu KTH,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1sm5h8r |
700 | 1 | a Lundin, Rickardu Swedish Institute of Space Physics, Kiruna4 aut |
700 | 1 | a Marklund, Göranu KTH,Rymd- och plasmafysik4 aut0 (Swepub:kth)u1yq52h6 |
700 | 1 | a Rathsman, Peteru Swedish Space Corporation, Solna, Sweden4 aut |
700 | 1 | a von Schéele, Fredriku Swedish Space Corporation, Solna, Sweden4 aut |
700 | 1 | a Wahlund, Jan-Eriku Swedish Institute of Space Physics, Uppsala4 aut |
710 | 2 | a Swedish Institute of Space Physics, Kirunab Swedish Institute of Space Physics, Uppsala4 org |
773 | 0 | t Proceedings of the 6th IAA International Conference on Low-Cost Planetary Missionsg , s. 227-232q <227-232 |
856 | 4 | u https://kth.diva-portal.org/smash/get/diva2:510817/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print |
856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-91583 |
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